Opening the window on strongly interacting dark matter

We discuss the possibility that the dark matter consists of strongly interacting massive particles (SIMP's) which have cross sections with ordinary matter which are larger than characteristic weak-interaction cross sections. We show that, while results from {beta}{beta} decay, cosmic-ray detect...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Veröffentlicht in:	Physical review. D, Particles and fields Particles and fields, 1990-06, Vol.41 (12), p.3594-3603
Hauptverfasser:	STARKMAN, G. D, GOULD, A, RAHIM ESMAILZADEH, DIMOPOULOS, S
Format:	Artikel
Sprache:	eng
Schlagworte:	645204 > High Energy Physics-- Particle Interactions & Properties-Theoretical-- Strong Interactions & Properties ANGULAR MOMENTUM BASIC INTERACTIONS BETA DECAY CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS COSMIC RAY DETECTION CROSS SECTIONS DECAY DETECTION ELEMENTS Exact sciences and technology Experimental studies of gravity GALAXIES General relativity and gravitation HYDROGEN INTERACTIONS MASS MEASURING INSTRUMENTS NEUTRON STARS NONLUMINOUS MATTER NONMETALS NUCLEAR DECAY PARTICLE PROPERTIES Physics PHYSICS OF ELEMENTARY PARTICLES AND FIELDS RADIATION DETECTION RADIATION DETECTORS SPIN STARS 640101 > Astrophysics & Cosmology-- Cosmic Radiation STRONG INTERACTIONS
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Schreiben Sie den ersten Kommentar!